www-hpcc.astro.washington.edu

University of Washington N-Body Shop Home Page

Computer Science and Engineering. Local HPCC Software Exchange Site. Click reload for new random picture. This interdisciplinary group led by Tom Quinn includes faculty and students from the departments of Astronomy. And Computer Science and Engineering. At the University of Washington. With support from the NSF. We also are collaborating with the Parallel Programming Laboratory. At the University of Illinois at Urbana-Champaign. On the development of Parallel tools for Cosmological N-body simulations.

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University of Washington N-Body Shop Home Page | www-hpcc.astro.washington.edu Reviews

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Computer Science and Engineering. Local HPCC Software Exchange Site. Click reload for new random picture. This interdisciplinary group led by Tom Quinn includes faculty and students from the departments of Astronomy. And Computer Science and Engineering. At the University of Washington. With support from the NSF. We also are collaborating with the Parallel Programming Laboratory. At the University of Illinois at Urbana-Champaign. On the development of Parallel tools for Cosmological N-body simulations.

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1 about us

2 contact info

3 university of washington

4 department of astronomy

5 department of physics

6 topics

7 participants

8 multimedia picture gallery

9 computing resources

10 graduate program

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University of Washington N-Body Shop Home Page | www-hpcc.astro.washington.edu Reviews

https://www-hpcc.astro.washington.edu

Computer Science and Engineering. Local HPCC Software Exchange Site. Click reload for new random picture. This interdisciplinary group led by Tom Quinn includes faculty and students from the departments of Astronomy. And Computer Science and Engineering. At the University of Washington. With support from the NSF. We also are collaborating with the Parallel Programming Laboratory. At the University of Illinois at Urbana-Champaign. On the development of Parallel tools for Cosmological N-body simulations.

INTERNAL PAGES

www-hpcc.astro.washington.edu

1

N-Body shop participants

http://www-hpcc.astro.washington.edu/participants.html

Search the Nasa Astrophysics Data. System for papers or preprints. Written by one of our participants. Computer Science and Engineering. Computer Science and Engineering. Computer Science and Engineering. Computer Science and Engineering. Derek C. Richardson. Frank van den Bosch. Seattle, WA 98195-1580. 206) 543-2888 voice, (206) 685-0403 FAX. Webmaster@www-hpcc.astro.washington.edu.

2

About N-Body shop

http://www-hpcc.astro.washington.edu/homepage/aboutus.html

Local HPCC Software Exchange Site. Recent Papers by the HPCC Group. Is part of the Department of Astronomy. At the University of Washington. We're in the business of designing and running software. That enables high-performance computing on a variety of astronomy-related problems, including large-scale structure formation and planet formation. Please feel free to explore the links on this website and learn more about our research! Seattle, WA 98195-1580. 206) 543-2888 voice, (206) 685-0403 FAX.

3

Software Tools

http://www-hpcc.astro.washington.edu/tools/tools.html

Contained here are the software tools developed by the NASA HPCC ESS group at the University of Washington. These tools may be freely obtained (see each tool for details) and used. The distribution of these tools are now hosted on our Github organization. If you have problems, questions or comments concerning this software, please submit an issue there. Massively parallel N-body/SPH solver. Parallel N-body visualization tool. Theoretical Image Processing System. Seattle, WA 98195-1580.

4

UW HPCC GROUP Picture Gallery

http://www-hpcc.astro.washington.edu/picture/picture.html

UW HPCC Group Picture Gallery. Recent Pictures/Movies By Topic. Most of the images in the Gallery were created with TIPSY. Face on view of a spiral galaxy similar to the Milky Way. This simulation took 100,000 CPU hours on the TACC Lonestar cluster. A very high-resolution simulation of the formation of a dark matter halo. To complete and will allow us to measure the density profile of a galaxy sized dark matter halo with unprecedented detail down to its very center. A simulation of a protoplanetary disk.

5

Computing Resources

http://www-hpcc.astro.washington.edu/resources.html

Most of our computing is performed at national centers. These include:. The National Center for Supercomputing Applications (NCSA). The Artic Region Supercomputing Center. The Pittsburgh Supercomputing Center. Thanks to a generous donation by Intel Corporation,. We have a 64 processor Pentium III Xeon Beowulf. It is located in the UW Center for Experimental Nuclear Physics and Astrophysics (CENPA). Gift also allowed us to purchase an SGI. Itanium cluster. Here are pictures of one. Seattle, WA 98195-1580.

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sixdayscience.com

Chapter 15 | SixDay Science

https://sixdayscience.com/curriculum/textbooks/chapter-15

Faith in Science Science in Faith. This chapter was copied with permission from Nick Strobel’s. Go to his site at www.astronomynotes.com. For the updated and corrected version. Other Galaxies and Active Galaxies. This chapter covers: the characteristics of other normal galaxies, active galaxies, and finding distances to other galaxies (this includes the distance-scale ladder). Also, large-scale structure is covered (galaxy clusters and collisions and superclusters). Edwin Hubble (courtesy of OCIW. Astron...

db.cs.washington.edu

AstroDB

http://db.cs.washington.edu/projects/astrodb.html

Astronomy has long been a data-intensive science. Today, the need to analyze massive amounts of data streaming from telescopes and generated by simulations is more pressing than ever. AstroDB is an inter-disciplinary group bringing together faculty from the department of Astronomy. In particular the Survey Science Group. And the N-body Shop. Department of Computer Science and Engineering. In particular the Database Group. And the UW eScience Instititute. Research Scientists and Faculty. SDSS image data i...

imp.mcmaster.ca

Gasoline Simulation Gallery

http://imp.mcmaster.ca/images

This is James Wadsley's. Gallery of images of the astrophysical simulations we are running at McMaster University. Using the computing resources of the SHARCNET collaboration ( www.sharcnet.ca. Some simulations shown were run elsewhere. The software we are using is the parallel SPH tree-code "Gasoline" developed at the University of Washington, "N-body Shop". By James Wadsley, Joachim Stadel and Tom Quinn. This paper. Dwarf Galaxies and the Destruction of Dark Matter Cusps. As recently presented in.

imp.mcmaster.ca

Software on Imp

http://imp.mcmaster.ca/software

Gasoline Parallel Tree-SPH code. Gasoline was developed within the University of Washington HPCC group. The main authors are James Wadsley, Joachim Stadel (Zurich) and Tom Quinn (Washington). The gasoline code is currently NOT public domain or otherwise generally available. Neither is the gravity code pkdgrav from which it was derived. We allow use of these codes outside the main coder group only as part of ongoing collaborations with the coders. HPCC University of Washington: Software Repository.

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www-hpcc.astro.washington.edu

University of Washington N-Body Shop Home Page

Computer Science and Engineering. Local HPCC Software Exchange Site. Click reload for new random picture. This interdisciplinary group led by Tom Quinn includes faculty and students from the departments of Astronomy. And Computer Science and Engineering. At the University of Washington. With support from the NSF. We also are collaborating with the Parallel Programming Laboratory. At the University of Illinois at Urbana-Champaign. On the development of Parallel tools for Cosmological N-body simulations.

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